Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment

O. Adriani; G. C. Barbarino; G. A. Bazilevskaya; R. Bellotti; M. Boezio; E. A. Bogomolov; M. Bongi; V. Bonvicini; S. Borisov; S. Bottai; A. Bruno; F. Cafagna; D. Campana; R. Carbone; P. Carlson; M. Casolino; G. Castellini; I. A. Danilchenko; M. P. De Pascale; C. De Santis; N. De Simone; V. Di Felice; V. Formato; A. M. Galper; A. V. Karelin; S. V. Koldashov; S. Koldobskiy; S. Y. Krutkov; A. N. Kvashnin; A. Leonov; V. Malakhov; L. Marcelli; A. G. Mayorov; W. Menn; V. V. Mikhailov; E. Mocchiutti; A. Monaco; N. Mori; N. Nikonov; G. Osteria; F. Palma; P. Papini; M. Pearce; P. Picozza; C. Pizzolotto; M. Ricci; S. B. Ricciarini; L. Rossetto; R. Sarkar; M. Simon; R. Sparvoli; P. Spillantini; Y. I. Stozhkov; A. Vacchi; E. Vannuccini; G. Vasilyev; S. A. Voronov; Y. T. Yurkin; J. Wu; G. Zampa; N. Zampa; V. G. Zverev

doi:10.1088/0004-637X/770/1/2

Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment

O. Adriani
, G. C. Barbarino
, G. A. Bazilevskaya
, R. Bellotti
, M. Boezio
, E. A. Bogomolov
, M. Bongi
, V. Bonvicini
, S. Borisov
, S. Bottai
, A. Bruno
, F. Cafagna
, D. Campana
, R. Carbone
, P. Carlson
, M. Casolino
, G. Castellini
, I. A. Danilchenko
, M. P. De Pascale
, C. De Santis

N. De Simone, V. Di Felice, V. Formato, A. M. Galper, A. V. Karelin, S. V. Koldashov, S. Koldobskiy, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, V. Malakhov, L. Marcelli, A. G. Mayorov, W. Menn, V. V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, N. Nikonov, G. Osteria, F. Palma, P. Papini, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, R. Sarkar, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, Y. T. Yurkin, J. Wu, G. Zampa, N. Zampa, V. G. Zverev

University of Florence
National Institute for Nuclear Physics
University of Naples Federico II
RAS - P.N. Lebedev Physics Institute
University of Bari
RAS - Ioffe Physico Technical Institute
University of Rome Tor Vergata
Moscow Engineering Physics Institute
AlbaNova University Center
RIKEN
National Research Council of Italy
University of Trieste
University of Siegen
Italian Space Agency

Research output: Contribution to journal › Article › peer-review

42 Scopus citations

Abstract

The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV/n for hydrogen and between 100 and 900 MeV/n for helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C.

Original language	English
Article number	2
Journal	Astrophysical Journal
Volume	770
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/770/1/2
State	Published - 10 Jun 2013
Externally published	Yes

Keywords

astroparticle physics
cosmic rays

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10.1088/0004-637X/770/1/2

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Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Danilchenko, I. A., De Pascale, M. P., ... Zverev, V. G. (2013). Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment. Astrophysical Journal, 770(1), Article 2. https://doi.org/10.1088/0004-637X/770/1/2

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abstract = "The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV/n for hydrogen and between 100 and 900 MeV/n for helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C.",

keywords = "astroparticle physics, cosmic rays",

author = "O. Adriani and Barbarino, \{G. C.\} and Bazilevskaya, \{G. A.\} and R. Bellotti and M. Boezio and Bogomolov, \{E. A.\} and M. Bongi and V. Bonvicini and S. Borisov and S. Bottai and A. Bruno and F. Cafagna and D. Campana and R. Carbone and P. Carlson and M. Casolino and G. Castellini and Danilchenko, \{I. A.\} and \{De Pascale\}, \{M. P.\} and \{De Santis\}, C. and \{De Simone\}, N. and \{Di Felice\}, V. and V. Formato and Galper, \{A. M.\} and Karelin, \{A. V.\} and Koldashov, \{S. V.\} and S. Koldobskiy and Krutkov, \{S. Y.\} and Kvashnin, \{A. N.\} and A. Leonov and V. Malakhov and L. Marcelli and Mayorov, \{A. G.\} and W. Menn and Mikhailov, \{V. V.\} and E. Mocchiutti and A. Monaco and N. Mori and N. Nikonov and G. Osteria and F. Palma and P. Papini and M. Pearce and P. Picozza and C. Pizzolotto and M. Ricci and Ricciarini, \{S. B.\} and L. Rossetto and R. Sarkar and M. Simon and R. Sparvoli and P. Spillantini and Stozhkov, \{Y. I.\} and A. Vacchi and E. Vannuccini and G. Vasilyev and Voronov, \{S. A.\} and Yurkin, \{Y. T.\} and J. Wu and G. Zampa and N. Zampa and Zverev, \{V. G.\}",

year = "2013",

month = jun,

day = "10",

doi = "10.1088/0004-637X/770/1/2",

language = "אנגלית",

volume = "770",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

}

Adriani, O, Barbarino, GC, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Danilchenko, IA, De Pascale, MP, De Santis, C, De Simone, N, Di Felice, V, Formato, V, Galper, AM, Karelin, AV, Koldashov, SV, Koldobskiy, S, Krutkov, SY, Kvashnin, AN, Leonov, A, Malakhov, V, Marcelli, L, Mayorov, AG, Menn, W, Mikhailov, VV, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, N, Osteria, G, Palma, F, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, SB, Rossetto, L, Sarkar, R, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, YI, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, SA, Yurkin, YT, Wu, J, Zampa, G, Zampa, N & Zverev, VG 2013, 'Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment', Astrophysical Journal, vol. 770, no. 1, 2. https://doi.org/10.1088/0004-637X/770/1/2

TY - JOUR

T1 - Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment

AU - Adriani, O.

AU - Barbarino, G. C.

AU - Bazilevskaya, G. A.

AU - Bellotti, R.

AU - Boezio, M.

AU - Bogomolov, E. A.

AU - Bongi, M.

AU - Bonvicini, V.

AU - Borisov, S.

AU - Bottai, S.

AU - Bruno, A.

AU - Cafagna, F.

AU - Campana, D.

AU - Carbone, R.

AU - Carlson, P.

AU - Casolino, M.

AU - Castellini, G.

AU - Danilchenko, I. A.

AU - De Pascale, M. P.

AU - De Santis, C.

AU - De Simone, N.

AU - Di Felice, V.

AU - Formato, V.

AU - Galper, A. M.

AU - Karelin, A. V.

AU - Koldashov, S. V.

AU - Koldobskiy, S.

AU - Krutkov, S. Y.

AU - Kvashnin, A. N.

AU - Leonov, A.

AU - Malakhov, V.

AU - Marcelli, L.

AU - Mayorov, A. G.

AU - Menn, W.

AU - Mikhailov, V. V.

AU - Mocchiutti, E.

AU - Monaco, A.

AU - Mori, N.

AU - Nikonov, N.

AU - Osteria, G.

AU - Palma, F.

AU - Papini, P.

AU - Pearce, M.

AU - Picozza, P.

AU - Pizzolotto, C.

AU - Ricci, M.

AU - Ricciarini, S. B.

AU - Rossetto, L.

AU - Sarkar, R.

AU - Simon, M.

AU - Sparvoli, R.

AU - Spillantini, P.

AU - Stozhkov, Y. I.

AU - Vacchi, A.

AU - Vannuccini, E.

AU - Vasilyev, G.

AU - Voronov, S. A.

AU - Yurkin, Y. T.

AU - Wu, J.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

PY - 2013/6/10

Y1 - 2013/6/10

N2 - The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV/n for hydrogen and between 100 and 900 MeV/n for helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C.

AB - The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV/n for hydrogen and between 100 and 900 MeV/n for helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C.

KW - astroparticle physics

KW - cosmic rays

UR - https://www.scopus.com/pages/publications/84878292345

U2 - 10.1088/0004-637X/770/1/2

DO - 10.1088/0004-637X/770/1/2

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:84878292345

SN - 0004-637X

VL - 770

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 2

ER -

Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment

Abstract

Keywords

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